Characteristics of field line resonance type geomagnetic pulsations and variations of plasmaspheric plasma density distribution

The period of field line resonance (FLR) type geomagnetic pulsations depends on the length of the field line and on the plasma density in the inner magnetosphere (plasmasphere), where field lines are closed. Here as FLR period, the period belonging to the maximum occurrence frequency of the occurrence frequency spectrum (equivalent resonance curve) of pulsations has been considered. The resonance system may be replaced by an equivalent resonant circuit. The plasma density would correspond to the ohmic load. The plasma in the plasmasphere originates from the ionosphere, thus FLR period, occurrence frequency are also affected by the maximum electron density in the ionosphere. The FLR period has shown an enhancement with increasing F region electron density, while the occurrence frequency indicated diminishing trend (possible damping effect). Thus, the increased plasma density may be the cause of the decreased occurrence of FLR type pulsations in the winter months of solar activity maximum years (winter anomaly).     

AEG评审在型号合格审定中的研究与应用

概述了申请人的航空器评审工作,并简要对比分析了运行符合性清单、型别等级和训练要求、MMEL、MRBR、OCAI等11个AEG工作评审项目。同时通过对比分析航空器评审组(简称AEG)评审与型号合格审定之间的区别和联系,为申请人顺利开展AEG工作提出4条建议。     

亚、跨、超声速下空腔流场特性实验研究

在FL-21跨、超声速风洞中对空腔流场特性进行了较为深入的实验研究.空腔的长深比L/D为7、8、9、12、15,试验马赫数M范围为0.6、0.9、1.2、1.5、1.8,试验雷诺数Re为1.23~2.26×107.研究表明:空腔流场特性主要由空腔长深比L/D和来流马赫数所决定,这两个参数的变化均能引起空腔的流场类型发生变化.另外,边界层厚度涠钥涨坏撞康难沽Ψ植家灿凶畔灾挠跋?随着边界层厚度与空腔深度之比?D的减小,空腔的流场类型有向闭式穴流动转变的趋势.     

Assessing ecohydrological factors variations and their relationships at different spatio-temporal scales in semiarid area,northwestern China

As a typical semiarid farming-pastoral ecotone sensitive to the environmennt, the Plain of West Liaohe Basin (WLBP) is currently experiencing drastic environmental changes. To identify how environmental change affect vegetation in the WLBP, we analysed spatiotemporal variation characteristics of Ecological environment factors based on monthly and annual air temperature (T), precipitation (P) and Normalized Difference Vegetation Index (NDVI) from 1982 to 2015. And the correlations between them were investigated by correlation analysis (Simple correlation, partial correlation and complex correlation) at temporal and spatial scale. The results showed that: (1) the vegetation growth of the WLBP showed ameliorated trend, with a change rate of 0.004/yr.; (2) P was more sensitive to NDVI than T; (3) and the influence of hydrothermal changes on vegetation growth was more significant than that of the change of single climate factors at time scales; (4) the effects of anthropogenic factors on vegetation change were 75.07% (1982–1993) and 98.08% (1994–2015), respectively. At the temp-special scales, P&T and land use type change (LUCC) were the main climatic and anthropogenic factors that affect vegetation changes, respectively.     

应用微机校定三相变压器的联结组及标号

三相变压的联结组标号对其正常运行极为重要，必须校定，而目前变还缺少全面快捷的校定方法和设备。本文介绍采用微机系统来实现联结组桔的校定，首先把四类联结组差别区分开，然后分析指出同一类联结组中，除有六种正序标号外，存在六种逆序标号，提出用新的筛选法能简捷地判别校定同一类的十二种标号，当微机系统进行实际测试时，必须考虑电源电压三相不对称程序的影响，故经数学推导得出用实测计算值代替理想计算值作判别比较的基     

Menger PM-空间上复合映射不动点定理的推广

设（X，F，△）和（Y，－↑F，△）是两个完备的MengerPM－空间，△是连续的H型t－范数，函数Φ（t）满足条件（Φ1)，本文在映射T：X→Y和S：Y→X满意更一般的条件下给出了关于复合映射TS和ST的不动点定理。这一定量进一步推广了Fisher,Sehgal和Bharucha-Reid等的有关结果，也是作者“MengerPM－空间上复合映射的不动点定理”一文的一般推广，最后给出了几个有用的结果作为本文主要定理的推广论。     

基于化学反应器网络模型法的预混气组分对NOx反应路径影响研究

摘 要：为探究预混气组分对不同反应路径下NOx生成影响,针对高压射流反应器,基于CFD流场特征等,构建优化了单PSR、2PSR、3PSR以及PSR+PFR四种化学反应器网络模型。在贫预混燃烧条件下,研究了纯CH4及其混合气燃烧时不同反应路径下NOx的生成情况,得出了燃烧室内不同反应区域每条反应路径NOx的生成量。结果表明,纯CH4燃烧产生的NOx主要来自于热力型、快速型和N2O-中间体型三条反应路径。绝热火焰温度的提高主要促进了热力型和N2O-中间体型NOx的生成。随着CH4或CO中加入H2摩尔分数的增加,NOx排放总量降低,快速型NOx生成速率降低,特别是火焰刷区域的。另外,混合气中CO摩尔分数的增加会导致NOx生成量增多。     

大型桥式机床立柱不同材料的特性分析

采用数值计算方法,比较了混凝土、铸铁和钢3种不同材料立柱的静载抗压能力以及冲击力下的瞬态响应,分析数据表明,钢立柱具有最好的承压能力,在相同压力下静变形最小;由于阻尼的原因,混凝土立柱的振幅受到明显限制,冲击力作用下振动衰减的较快,在更加关注减振性能的高速高性能加工领域,采用混凝土立柱是更好的选择.     

开环全保偏光纤陀螺研究

开环全保偏光纤陀螺结构简单，有使用价值；进入９０年代国外研究成功熔接型保偏光纤耦合器以后，这种陀螺更受重视，向实用方向发展，对研究全保偏光纤陀螺中的几个关键问题，光路中元器件的特性；保偏光纤的对轴熔接技术，零漂和噪声做了分析，实验结果表明，零漂达到１．２４°／ｈ。     

LMXB luminosity function and connection to globular cluster in early type galaxies

We derive bias-corrected X-ray luminosity functions (XLFs) of LMXBs detected in 14 E and S0 galaxies observed with Chandra. After correcting for incompleteness, the individual XLFs are statistically consistent with a single power-law. A break at or near L_X,Eddington , as previously reported, is not required in any individual case. The combined XLF with a reduced error, however, suggests a possible break at L_X = 5 × 10³⁸ erg s⁻¹, which may be consistent with the Eddington luminosity of neutron stars with the largest possible mass (3 M), or of He-enriched neutron star binaries. We confirm that the total X-ray luminosity of LMXBs is correlated with the the near-IR luminosities, but the scatter exceeds that expected from measurement errors. The scatter in L_X(LMXB)/L_K appears to be correlated with the specific frequency of globular clusters, as reported earlier.

We cross-correlate X-ray binaries with globular clusters determined by ground-based optical and HST observations in 6 giant elliptical galaxies. With the largest sample reported so far (300 GC LMXBs with a 5:2 ratio between red and blue GCs), we compare their X-ray properties, such as X-ray hardness, XLF and L_X/L_B and find no statistically significance difference between different groups of LMXBs. Regardless of their association with GCs, both GC and field LMXBs appear to follow the radial profile of the optical halo light, rather than that of more extended GCs. This suggests that while metallicity is a primary factor in the formation of LMXBs in GCs, there may be a secondary factor (e.g., encounter rate) playing a non-negligible role.